THE FILAMENTS OF NGC-1275 - A COLLISION BETWEEN A GALAXY AND AN ACCRETION FLOW

被引：49

作者：

HU, EM

COWIE, LL

KAARET, P

JENKINS, EB

YORK, DG

ROESLER, FL

机构：

[1] NASA,GODDARD SPACE FLIGHT CTR,HIGH ENERGY ASTROPHYS LAB,GREENBELT,MD 20771

[2] MIT,DEPT PHYS,CAMBRIDGE,MA 02139

[3] PRINCETON UNIV OBSERV,PRINCETON,NJ 08544

[4] UNIV WISCONSIN,DEPT PHYS,MADISON,WI 53706

[5] UNIV MARYLAND,DEPT PHYS & ASTRON,COLLEGE PK,MD 20742

[6] MIT,CTR SPACE RES,CAMBRIDGE,MA 02139

[7] MIT,CTR THEORET PHYS,CAMBRIDGE,MA 02139

来源：

ASTROPHYSICAL JOURNAL | 1983年 / 275卷 / 02期

关键词：

D O I：

10.1086/184165

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L27 / &

共 17 条

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[6] THE DISTRIBUTION AND MORPHOLOGY OF X-RAY-EMITTING GAS IN THE CORE OF THE PERSEUS CLUSTER [J].

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[7] TIME VARIATIONS OF THE NEUTRAL HYDROGEN ABSORPTION-SPECTRUM OF NGC-1275 (3C 84) [J].

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[8] OPTICAL EMISSION-LINE GAS ASSOCIATED WITH DOMINANT CLUSTER GALAXIES [J].

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[9] IONIZATION AND EXCITATION MECHANISMS IN THE FILAMENTS AROUND NGC-1275 [J].

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[10]

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